SDO HMI 2014-11-26 00:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.22 | 346.55 | 148.51 | 836.78 | -15.55 | 243.13 | 76.91 | 253.67 | 0.9764 | -297.4 | -57.8 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.28 | 26.37 | 44.41 | 168.09 | -12.85 | 251.08 | 84.86 | 256.97 | 0.9971 | -14.5 | 121.1 | |
| 0.00 | 1.03 | 0.00 | 2.17 | -11.86 | 241.99 | 75.77 | 257.40 | 0.9731 | 158.0 | 135.8 | |
| 0.00 | 2.14 | 0.00 | 4.37 | -12.85 | 241.48 | 75.26 | 256.34 | 0.9714 | -351.0 | -247.9 | |
| 4.62 | 316.58 | 9.54 | 661.33 | -14.51 | 241.44 | 75.22 | 254.64 | 0.9718 | -579.2 | -96.3 | |
| 1.97 | -4.00 | 4.32 | -4.00 | -15.24 | 242.21 | 75.98 | 253.97 | 0.9750 | -306.0 | 999999 | |
| 4.45 | -4.00 | 9.75 | -4.00 | -15.48 | 242.22 | 76.00 | 253.72 | 0.9752 | -347.5 | 999999 | |
| 2.57 | -4.00 | 5.15 | -4.00 | -14.86 | 240.95 | 74.73 | 254.23 | 0.9700 | -571.4 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.82 | -14.91 | 240.30 | 74.07 | 254.12 | 0.9673 | -434.0 | -382.0 | |
| 4.37 | -4.00 | 8.61 | -4.00 | -15.66 | 240.69 | 74.47 | 253.39 | 0.9693 | -222.6 | 999999 | |
| 23.03 | -4.00 | 48.49 | -4.00 | -16.95 | 241.50 | 75.28 | 252.15 | 0.9730 | -299.2 | 999999 | |
| 9.93 | -4.00 | 18.24 | -4.00 | -16.74 | 239.42 | 73.19 | 252.14 | 0.9644 | -777.7 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |